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Stellar HostProfile

Kepler-373

Unclassified star • 1090.5 pc

Records

22

literature rows

Planets

2

system count

References

16

distinct source labels

TIC: TIC 299218776

Approximate color

from effective temperature

Canonical Summary

Adopted host values from one source row

Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.

Stellar source: Morton et al. 2016 • System source: TICv8

Temperature

5595 K

5410.7 to 5803

20 values • 9 distinct

Mass

0.93 Msun

0.87 to 0.98

14 values • 7 distinct

Radius

0.90 Rsun

0.80 to 1.42

20 values • 11 distinct

Age

4.17 Gyr

0.50 to 10.96

4 values • 3 distinct

Distance

1090.5 pc

single adopted value

22 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.90 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Kepler-373

0.90 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2014

Period

5.54 days

Radius

1.36 R⊕

Mass

—

Eq. Temp

—

◌

Discovery

2014

Period

16.73 days

Radius

1.24 R⊕

Mass

—

Eq. Temp

—

Kepler-373 and Its Two Planets

Kepler-373 is a star located 3560 light-years away. It hosts two planets, both discovered by transit in 2014. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness; repeated dips help establish orbital periods. The star's reported mass estimate is smaller than the Sun's, and its reported temperature of 5600 K is cooler than the Sun's. It is 0.93 solar masses, 0.9 solar radii, and 4.17 billion years old.

Kepler-373 b and Kepler-373 c are both Earth-like planets, a size class that stays within 1.5 times Earth's radius. Kepler-373 b has an orbital period of 5.54 days and a radius of 1.36 Earth radii. Kepler-373 c orbits every 16.7 days at 1.24 Earth radii. Among the listed planets, Kepler-373 b has the shortest year by reported estimates, while Kepler-373 c has the longest. Kepler-373 b also has the largest radius by reported estimates, and Kepler-373 c the smallest.

Provenance

Underlying measurements and references

Evidence Summary

Rows

22

Stellar refs

15

System refs

1

Distancestable

22 values • 1 distinct

Parallaxstable

22 values • 1 distinct

Temperaturedisputed

20 values • 9 distinct

Massdisputed

14 values • 7 distinct

Radiusdisputed

20 values • 11 distinct

Agedisputed

4 values • 3 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

17 values • 7 distinct

Metallicitydisputed

12 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
57830.900.84———1090.5Q1-Q17 DR24 KOI TableTICv8
58030.980.870.50——1090.5Q1-Q8 KOI TableTICv8
58030.980.870.50——1090.5Q1-Q8 KOI TableTICv8
57830.900.84———1090.5Q1-Q12 KOI TableTICv8
55530.981.38—0.21—1090.5TICv8TICv8
——————1090.5Q1-Q17 DR25 Supplemental KOI TableTICv8
55880.951.10———1090.5Q1-Q17 DR25 KOI TableTICv8
55390.870.80———1090.5Batalha et al. 2013TICv8
5539—0.80———1090.5Q1-Q6 KOI TableTICv8
——————1090.5Q1-Q17 DR25 Supplemental KOI TableTICv8
5539—0.87———1090.5Latham et al. 2005TICv8
57830.900.84———1090.5Q1-Q17 DR24 KOI TableTICv8
5539—0.80———1090.5Q1-Q6 KOI TableTICv8
5410.7—1.42—0.19—1090.5Gaia DR2TICv8
57830.900.84———1090.5Q1-Q16 KOI TableTICv8
57830.900.84———1090.5Q1-Q12 KOI TableTICv8
57830.900.84———1090.5Q1-Q16 KOI TableTICv8
55950.930.904.17——1090.5Morton et al. 2016TICv8
56020.981.3310.96——1090.5Fulton & Petigura 2018TICv8
5602—1.36———1090.5Berger et al. 2018TICv8
55880.951.10———1090.5Q1-Q17 DR25 KOI TableTICv8
5787—0.84———1090.5Rowe et al. 2014TICv8